MRC B1221-423: Forming an AGN in a merger

Details MRC B1221-423: Forming an AGN in a merger MRC B1221-423: Forming an AGN in a merger

Nov 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004iaus..222..451j&link_type=abstract

The Interplay among Black Holes, Stars and ISM in Galactic Nuclei, Proceedings of IAU Symposium, No. 222. Edited by T. Storchi-B

Computer Science

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Scientific paper

MRC B1221-423 is a powerful, nearby (z = 0.17) compact radio source, which lies within the envelope of a galaxy which is undergoing a tidal interaction with a companion. Broad-band optical/NIR colours show evidence of several distinct episodes of star formation. The evidence points to this being a radio source `caught in the act' of its first ignition.

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